output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2012 · astro-ph.EPShow all

11 papers · 2 filters

astro-ph.EP2012★ 29 cited

WASP-71b: a bloated hot Jupiter in a 2.9-day, prograde orbit around an evolved F8 star

A. M. S. Smith, D. R. Anderson, F. Bouchy +20

We report the discovery by the WASP transit survey of a highly-irradiated, massive (2.242 +/- 0.080 MJup) planet which transits a bright (V = 10.6), evolved F8 star every 2.9 days.…

astro-ph.EP2012★ 74 cited

The thermal reactivity of HCN and NH3 in interstellar ice analogues

J. A. Noble, P. Theule, F. Borget +5

HCN is a molecule central to interstellar chemistry, since it is the simplest molecule containing a carbon-nitrogen bond and its solid state chemistry is rich. The aim of this work…

astro-ph.EP2012★ 114 cited

A Gas Giant Circumbinary Planet Transiting the F Star Primary of the Eclipsing Binary Star KIC 4862625 and the Independent Discovery and Characterization of the two transiting planets in the Kepler-47 System

Veselin B. Kostov, Peter McCullough, Tobias Hinse +5

We report the discovery of a transiting, gas giant circumbinary planet orbiting the eclipsing binary KIC 4862625 and describe our independent discovery of the two transiting planet…

astro-ph.EP2012★ 25 cited

Detection of Neptune-size planetary candidates with CoRoT data. Comparison with the planet occurrence rate derived from Kepler

Aldo S. Bonomo, Pierre-Yves Chabaud, Magali Deleuil +10

[Abridged] Context. The CoRoT space mission has been searching for transiting planets since the end of December 2006. Aims. We aim to investigate the capability of CoRoT to detect…

astro-ph.EP2012★ 10 cited

A long-period massive planet around HD106515A

S. Desidera, R. Gratton, E. Carolo +9

We have performed RV monitoring of the components of the binary system HD 106515 over about 11 years using the high resolution spectrograph SARG at TNG. The primary shows long-peri…

astro-ph.EP2012★ 41 cited

SOPHIE velocimetry of Kepler transit candidates VI. An additional companion in the KOI-13 system

A. Santerne, C. Moutou, S. C. C. Barros +7

We report the discovery of a new stellar companion in the KOI-13 system. KOI-13 is composed by two fast-rotating A-type stars of similar magnitude. One of these two stars hosts a t…

astro-ph.EP2012★ 44 cited

Doppler tomography of transiting exoplanets: A prograde, low-inclined orbit for the hot Jupiter CoRoT-11b

Davide Gandolfi, Andrew Collier Cameron, Michael Endl +8

We report the detection of the Doppler shadow of the transiting hot Jupiter CoRoT-11b. Our analysis is based on line-profile tomography of time-series, Keck/HIRES high-resolution s…

astro-ph.EP2012★ 82 cited

The Bimodal Colors of Centaurs and Small Kuiper Belt Objects

Nuno Peixinho, Audrey Delsanti, Aurélie Guilbert-Lepoutre +2

Ever since the very first photometric studies of Centaurs and Kuiper Belt Objects (KBOs) their visible color distribution has been controversial. That controversy gave rise to a pr…

astro-ph.EP2012★ 183 cited

SOPHIE velocimetry of Kepler transit candidates VII. A false-positive rate of 35% for Kepler close-in giant exoplanet candidates

A. Santerne, R. F. Díaz, C. Moutou +6

The false-positive probability (FPP) of Kepler transiting candidates is a key value for statistical studies of candidate properties. A previous investigation of the stellar populat…

astro-ph.EP2012★ 79 cited

Elliptical instability in terrestrial planets and moons

David Cébron, Michael Le Bars, Claire Moutou +1

The presence of celestial companions means that any planet may be subject to three kinds of harmonic mechanical forcing: tides, precession/nutation, and libration. These forcings c…

astro-ph.EP2012★ 33 cited

Transiting exoplanets from the CoRoT space mission XXI. CoRoT-19b: A low density planet orbiting an old inactive F9V-star

E. W. Guenther, R. F. Diaz, J. -C. Gazzano +51

Observations of transiting extrasolar planets are of key importance to our understanding of planets because their mass, radius, and mass density can be determined. The CoRoT space…